Understanding the climates of terrestrial exoplanets and the detectability of biosignatures is an inherently interdisciplinary challenge, requiring the integration of insights from Solar System exploration, exoplanet observations and climate science. […]
astro-ph.EP
Spatial Distribution Of Organics In The Horsehead Nebula: Signposts Of Chemistry Driven By Atomic Carbon
(Abridged) Complex organic molecules (COMs) are considered essential precursors to prebiotic species. While COMs were once expected to be efficiently destroyed under UV-irradiated conditions, detections in photodissociation regions (PDRs) have […]
The RoPES Project With HARPS and HARPS-N II. A Third Planet In The Multi-planet System HD 176986
Context. Earth-like planets orbiting in the habitable zone of K- to G-type stars create an RV effect in amplitude of less than 1 m s−1 and have orbital periods of […]
H182O In The Terrestrial Planet-forming Regions Of Protoplanetary Disks
Isotopologues play an important role in solar system cosmochemistry studies, revealing details of early planet formation physics and chemistry.
Orbital Stability Of Compact Three-planet Systems III. The Role Of Three-body Resonances
Observational surveys show that at least ~ 30% of short-period multiplanetary systems host tightly packed planets, some of which are locked in stable chains of mean-motion resonances.
Discovery and Characterisation of Two Exoplanets Orbiting the Metal-poor, Solar-type Star TOI-5788 with TESS, CHEOPS, and HARPS-N
We present the discovery and characterisation of two transiting exoplanets orbiting the metal-poor, solar-type star TOI-5788.
Orbital Stability Of Closely-Spaced Four-planet Systems
We investigate the orbital dynamics of four-planet systems consisting of Earth-mass planets on initially-circular, coplanar orbits around a star of one solar mass.
A Cool Earth-sized Planet Candidate Transiting a Tenth Magnitude K-dwarf From K2
The transit method is currently one of our best means for the detection of potentially habitable “Earth-like” exoplanets.
Possible Favored Great Oxidation Event Scenario On Exoplanets Around M-Stars With The Example Of TRAPPIST-1e
The Great Oxidation Event (GOE), which marked the transition from an anoxic to an oxygenated atmosphere, occurred 2.4 billion years ago on Earth, several hundreds of millions of years after […]
Modeling the Impact of Unresolved Stellar Companions on Detection Sensitivity in Kepler’s Small Planet Occurrence Rates
Unresolved stellar companions can cause both under-estimations in the radii of transiting planets and over-estimations of their detectability, affecting our ability to reliably measure planet occurrence rates.
